The abstract you have submited
HIGH ENERGY NEUTRAL EMISSIONS OF LARGE SOLAR FLARES IN THE END OF OCTOBER, 2003.
Kuznetsov S.N., Kurt V.G., Myagkova I.N., Yushkov B.Yu., Kudela K.,
This report is a description for the large solar flares detected with the spectrometer (SONG) on the CORONAS-F mission during famous period of solar activity in the end of October 2003. The intensive gamma-emission were detected during the impulsive phase of two flares from active region NOAA 0486 - October 28 (11:02-11:13 UT, è17.2/4B, S16E08 ) and October 29 (20:38-20:55 UT, X10/2B, S15W02). The basic scientific data from SONG consist of the counting rate recorded every 4s in each of channels in energy interval 50 keV - 100 MeV. Comparison of the Hard X-ray and gamma-ray emission time behavior with the main SXR source characteristics such a temperature, emission measure and energy injection function G(t) was made. In addition we compared the Neupert's derivative and the energy injection function G(t) with the flux of the 150 keV X-rays, registered by SONG spectrometer to define how the very intense high energy electrons beam deposits its energy into SXR source.